基站天线异常贝塞尔-汉克尔场的特异吸收辐射测量

H. Nieto-Chaupis
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引用次数: 1

摘要

本文主要研究基站天线附近发射功率不超过已知辐射标准和规范要求的异常场的识别和计算。为此,利用源的各向同性场发射,将经典势向量的指数部分展开为球面汉克尔函数和贝塞尔函数。高次谐波在计算中的应用是本工作的重点。为了观察异常场,在所有电动力学关系中加入了多达25个谐波。我们将自己重新连接到那些基站天线,这些天线位于5至10米高的建筑物上。在这项研究中发现,通过测量特定吸收辐射(SAR),所提出的公式与暴露水平标准值的偏差可以忽略不计,从而排除了辐射源周围辐射污染的可能性。目前的模型与以前的工作相比产生了2.5%的差异,这一事实是在2GHz和1 Vm-1源的SAR值约为24μWKg-1的情况下,考虑到0.5%的数量级误差。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Specific absorption radiation measurement of anomalous Bessel-Hankel fields by base stations antennas
This paper focuses on the identification and calculation of anomalous fields in the vicinity of base stations antennas whose power emission does not surpasses the required ones as dictated by the well-known radiation standards and norms. For this end, the exponential part of the classical potential vector is expanded onto spherical Hankel and Bessel functions by taking advantage of the isotropic field emission of the source. The usage of high harmonics in the calculations is the key point in this work. In order to observe anomalous field, up to 25 harmonics in all electrodynamics relations were added. We restring ourselves to those base stations antennas located on buildings whose height are ranging between 5 and 10 m. In this study is encountered that the proposed formulation yields a negligible deviation from standard values of exposure levels, through the measurement of specific absorption radiation (SAR) thereby discarding possibilities of contamination by radiation around the emission source. The present model yields a difference of 2.5% with respect to previous works, fact which is traduced in SAR values of around 24μWKg-1 for a 2GHz and 1 Vm-1 source, contemplating an error of order of 0.5%.
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